与Lherz橄榄岩体接触的含蓝宝石岩石:新的矿物学资料、年龄和解释

Jessica Uzel, Y. Lagabrielle, S. Fourcade, C. Chopin, P. Monchoux, C. Clerc, M. Poujol
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引用次数: 3

摘要

在法国的Aulus盆地(ari法兰西),在Lherz橄榄岩体和中生代变质沉积层的接触带中发现了含蓝宝石的岩石(Monchoux, 1970,1972a, 1972b),这些变质沉积层经历了比利牛斯白垩纪高温低压变质事件。蓝宝石晶体出现在层状碎屑矿床中,其特征是一套罕见的富铝镁矿物。本文对16个样品进行了详细的岩石学研究,这些样品代表了Lherz含蓝宝石岩石的多样性。这些岩石包括角砾岩和微角砾岩,其成分各不相同。一些样品由多矿物碎屑和分离矿物组成,这些矿物来自于区域知名的原岩,如超镁铁质岩石、变质岩、“云母角砾岩”和非常稀少的古生代基底岩。然而,大部分含蓝宝石碎屑套是由来自未知原岩的单矿物和多矿物碎屑组成的。我们定义了一个“含蓝宝石矿物套”(SBMS),由单矿物碎屑组成,包括:蓝宝石+顽辉石+铝尖晶石+镁角闪石+钙角闪石+角闪石+辅助矿物(磷灰石、透辉石、金红石、蛇纹石、蒙脱石、电气石、蛭石和白色云母)。我们在研究的岩石中强调了变质的Keuper碎屑物质的优势,并且在富al - mg套件的矿物中存在硬石膏和富F, Cl-, sr的磷灰石包裹体。角砾质结构和明确的沉积特征表明,含蓝宝石岩石在水下条件下经历了机械分解和筛分,不同来源之间的混合很差。我们测量了U-Pb金红石年龄数据,以便对这些碎屑矿床的原岩年龄提供约束。得到的年龄(98.6 + 1.2 Ma)被解释为该SBMS原岩的变质年龄。以前的研究将Lherz含蓝宝石岩石解释为地壳原岩,在与Lherz体的超镁质岩石接触的过程中,地壳原岩在深度上发生了改变,并向较浅的深度上升。这些新资料表明:(1)含蓝宝石岩石的主要原岩起源于上三叠统至下侏罗统;(ii)该原岩在塞诺曼期沿活跃的热壳幔分离作用变质,并有交代的咸水型流体参与;(3)由于拆离作用的演化,在挖掘过程中发生角化作用,随后对变质物质进行沉积改造。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The sapphirine-bearing rocks in contact with the Lherz peridotite body: New mineralogical data, age and interpretation
Sapphirine-bearing rocks are described in the Aulus Basin (Ariège, France) in a contact zone between the Lherz peridotitic body and Mesozoic metasediments which underwent the Pyrenean Cretaceous high-temperature, low-pressure metamorphic event (Monchoux, 1970, 1972a, 1972b). Sapphirine crystals occur in layered clastic deposits characterized by an uncommon suite of Al-Mg-rich minerals. A detailed petrographic study of sixteen samples representative of the diversity of the Lherz sapphirine-bearing rocks is presented. These rocks include breccias and microbreccias with various compositions. Some samples are composed of polymineralic clasts and isolated minerals that derive from regionally well-known protoliths such as ultramafic rocks, meta-ophites, “micaceous hornfels”, and very scarce Paleozoic basement rocks. Nevertheless, a large portion of the sapphirine-bearing clastic suite is composed of mono- and polymineralic debris that derive from unknown protolith(s). We define a "sapphirine-bearing mineral suite” (SBMS) composed of monomineralic debris including: sapphirine + enstatite + aluminous spinel + Mg-amphiboles + Ca-amphiboles + kornerupine + accessory minerals (apatite, diopside, rutile, serpentine, smectite, tourmaline, vermiculite and a white mica). We highlight the dominance of metamorphic Keuper clastic materials in the studied rocks and the presence of inclusions of anhydrite and F-, Cl-, Sr-rich apatite in minerals of the Al-Mg-rich suite. The brecciated texture and the presence of unequivocal sedimentary features suggest that the sapphirine-bearing rocks were mechanically disaggregated and then experienced winnowing in underwater conditions with poor mixing between the different sources. We measured U-Pb rutile age data in order to provide constraints on the age of (one of) the protolith(s) of those clastic deposits. The obtained age (98.6 + 1.2 Ma) is interpreted as the age of metamorphism of this protolith of the SBMS. Previous works interpreted the Lherz sapphirine-bearing rocks as crustal protoliths modified at depth along the contact with the ultramafic rocks of the Lherz body during their ascent towards shallower depths. These new data imply: (i) an Upper Triassic to Lower Jurassic origin for the main protolith of the sapphirine-bearing rocks; (ii) the metamorphism of this protolith along an active hot crust–mantle detachment during Cenomanian times with the involvement of metasomatic, brine-type fluids; and (iii) its brecciation during the exhumation of the material due to the evolution of the detachment, followed by subsequent sedimentary reworking of the metamorphic material.
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